! Started logfile: J0239+0416_X_2003_06_18_pus_uvs.log on Wed Jan 17 16:15:58 2007 obs J0239+0416_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J0239+0416_X_2003_06_18_pus_uva.fits ! AN table 1: 204 integrations on 153 of 153 possible baselines. ! AN table 2: 119 integrations on 153 of 153 possible baselines. ! AN table 3: 125 integrations on 153 of 153 possible baselines. ! AN table 4: 24 integrations on 153 of 153 possible baselines. ! AN table 5: 98 integrations on 153 of 153 possible baselines. ! AN table 6: 363 integrations on 153 of 153 possible baselines. ! AN table 7: Unused. ! AN table 8: Unused. ! AN table 9: Unused. ! Apparent sampling: 0.0889113 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0239+0416 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2231 lines of history. ! ! Reading 50768 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 float field_size field_size = 256 float field_cell field_cell = 0.2 float taper_size taper_size = 70. integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 256x256 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 2965 telescope corrections were flagged in sub-array 1. ! A total of 1752 telescope corrections were flagged in sub-array 2. ! A total of 2202 telescope corrections were flagged in sub-array 3. ! A total of 275 telescope corrections were flagged in sub-array 4. ! A total of 1691 telescope corrections were flagged in sub-array 5. ! A total of 5997 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 2776 telescope corrections were flagged in sub-array 1. ! A total of 1752 telescope corrections were flagged in sub-array 2. ! A total of 2154 telescope corrections were flagged in sub-array 3. ! A total of 275 telescope corrections were flagged in sub-array 4. ! A total of 1640 telescope corrections were flagged in sub-array 5. ! A total of 5997 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 2777 telescope corrections were flagged in sub-array 1. ! A total of 1752 telescope corrections were flagged in sub-array 2. ! A total of 2154 telescope corrections were flagged in sub-array 3. ! A total of 275 telescope corrections were flagged in sub-array 4. ! A total of 1640 telescope corrections were flagged in sub-array 5. ! A total of 5997 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 2777 telescope corrections were flagged in sub-array 1. ! A total of 1752 telescope corrections were flagged in sub-array 2. ! A total of 2154 telescope corrections were flagged in sub-array 3. ! A total of 275 telescope corrections were flagged in sub-array 4. ! A total of 1640 telescope corrections were flagged in sub-array 5. ! A total of 5997 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=0.843682Jy sigma=0.008411 ! Fit after self-cal, rms=0.596050Jy sigma=0.005756 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.863% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! The y-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.5544 mas, bmaj=1.808 mas, bpa=-4.556 degrees ! Estimated noise=702.62 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.377937 Jy ! Component: 100 - total flux cleaned = 0.479884 Jy ! Total flux subtracted in 100 components = 0.479884 Jy ! Clean residual min=-0.011775 max=0.043584 Jy/beam ! Clean residual mean=0.000834 rms=0.004651 Jy/beam ! Combined flux in latest and established models = 0.479884 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.479884 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.380091Jy sigma=0.002188 ! Fit after self-cal, rms=0.379828Jy sigma=0.002186 ! Inverting map ! Your choice of large map pixels excluded 0.863% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! The y-axis pixel size should ideally be below 0.1974 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0468269 Jy ! Component: 100 - total flux cleaned = 0.0712771 Jy ! Total flux subtracted in 100 components = 0.0712771 Jy ! Clean residual min=-0.008754 max=0.021348 Jy/beam ! Clean residual mean=0.000452 rms=0.003100 Jy/beam ! Combined flux in latest and established models = 0.551161 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 21 components and 0.551162 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.370843Jy sigma=0.001918 ! Fit after self-cal, rms=0.370692Jy sigma=0.001918 ! Inverting map ! Your choice of large map pixels excluded 0.863% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! The y-axis pixel size should ideally be below 0.1974 milli-arcsec ! Added new window around map position (-1.4, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0212523 Jy ! Component: 100 - total flux cleaned = 0.0352752 Jy ! Total flux subtracted in 100 components = 0.0352752 Jy ! Clean residual min=-0.008340 max=0.009919 Jy/beam ! Clean residual mean=0.000274 rms=0.002588 Jy/beam ! Combined flux in latest and established models = 0.586437 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 30 components and 0.586437 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.368627Jy sigma=0.001850 ! Fit after self-cal, rms=0.368622Jy sigma=0.001847 ! Inverting map ! Your choice of large map pixels excluded 0.863% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! The y-axis pixel size should ideally be below 0.1974 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.863% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! The y-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.7613 mas, bmaj=2.223 mas, bpa=-8.985 degrees ! Estimated noise=459.137 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0210618 Jy ! Component: 100 - total flux cleaned = 0.0315786 Jy ! Component: 150 - total flux cleaned = 0.037345 Jy ! Component: 200 - total flux cleaned = 0.040694 Jy ! Total flux subtracted in 200 components = 0.040694 Jy ! Clean residual min=-0.007893 max=0.007642 Jy/beam ! Clean residual mean=0.000642 rms=0.002056 Jy/beam ! Combined flux in latest and established models = 0.627131 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 44 components and 0.627131 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.367615Jy sigma=0.001813 ! Fit after self-cal, rms=0.367528Jy sigma=0.001811 ! Inverting map ! Your choice of large map pixels excluded 0.863% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! The y-axis pixel size should ideally be below 0.1974 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 102 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 0.93 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* ON 1.05 OV 1.00* ! PT 1.00* SC 1.01 TC 1.00* TS 1.00* ! WF 0.97 WZ 1.03 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.97 GG 1.00* HN 1.08 ! KK 1.08 KP 0.96 LA 0.99 MA 1.00* ! MK 0.98 NL 1.05 ON 1.00* OV 0.97 ! PT 1.00 SC 1.01 TC 1.00* TS 1.05 ! WF 1.13 WZ 1.04 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.97 GG 1.00* HN 1.01 ! KK 1.00* KP 1.02 LA 0.97 MA 1.00* ! MK 1.00* NL 1.05 ON 1.00* OV 0.98 ! PT 0.99 SC 1.01 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.16 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 0.95 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.27 ON 1.00* OV 1.00* ! PT 1.00* SC 1.02 TC 1.00* TS 1.00* ! WF 1.00* WZ 0.97 ! ! A total of 138 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.98 GG 1.00* HN 0.96 ! KK 1.00* KP 1.02 LA 0.98 MA 1.00* ! MK 1.00* NL 1.05 ON 1.00* OV 0.99 ! PT 0.97 SC 1.04 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 0.96 ! KK 1.00* KP 1.00* LA 1.00* MA 1.07 ! MK 1.00* NL 1.00* ON 1.04 OV 1.00* ! PT 1.00* SC 0.96 TC 1.00* TS 1.00* ! WF 0.98 WZ 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.96 GG 1.00* HN 1.06 ! KK 1.06 KP 0.92 LA 0.97 MA 1.00* ! MK 0.98 NL 1.02 ON 1.00* OV 0.97 ! PT 1.04 SC 1.00 TC 1.00* TS 1.01 ! WF 1.17 WZ 0.92 ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.95 GG 1.00* HN 1.01 ! KK 1.00* KP 0.95 LA 0.95 MA 1.00* ! MK 1.00* NL 1.03 ON 1.00* OV 0.96 ! PT 1.02 SC 1.01 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.09 ! ! A total of 60 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 1.02 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.08 ON 1.00* OV 1.00* ! PT 1.00* SC 1.03 TC 1.00* TS 1.00* ! WF 1.00* WZ 0.93 ! ! A total of 138 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.96 GG 1.00* HN 0.94 ! KK 1.00* KP 0.97 LA 0.98 MA 1.00* ! MK 1.00* NL 1.00 ON 1.00* OV 1.00 ! PT 1.02 SC 1.01 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 0.95 ! KK 1.00* KP 1.00* LA 1.00* MA 1.04 ! MK 1.00* NL 1.00* ON 1.01 OV 1.00* ! PT 1.00* SC 0.96 TC 1.00* TS 1.00* ! WF 0.89 WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 0.95 GG 1.00* HN 1.07 ! KK 1.13 KP 0.96 LA 0.97 MA 1.00* ! MK 1.00 NL 1.02 ON 1.00* OV 1.01 ! PT 1.08 SC 1.04 TC 1.00* TS 1.00 ! WF 1.04 WZ 0.91 ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 0.96 GG 1.00* HN 0.99 ! KK 1.00* KP 0.98 LA 0.97 MA 1.00* ! MK 1.00* NL 0.99 ON 1.00* OV 1.01 ! PT 1.06 SC 1.00 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.14 ! ! A total of 60 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 1.03 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.09 ON 1.00* OV 1.00* ! PT 1.00* SC 1.03 TC 1.00* TS 1.00* ! WF 1.00* WZ 0.90 ! ! A total of 138 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 0.96 GG 1.00* HN 0.93 ! KK 1.00* KP 1.01 LA 1.00 MA 1.00* ! MK 1.00* NL 1.00 ON 1.00* OV 1.03 ! PT 1.04 SC 0.96 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00 ! KK 1.00* KP 1.00* LA 1.00* MA 0.96 ! MK 1.00* NL 1.00* ON 1.13 OV 1.00* ! PT 1.00* SC 1.04 TC 1.00* TS 1.00* ! WF 0.89 WZ 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.95 GG 1.00* HN 1.13 ! KK 1.09 KP 0.93 LA 0.96 MA 1.00* ! MK 1.01 NL 1.02 ON 1.00* OV 1.00 ! PT 1.07 SC 1.05 TC 1.00* TS 0.99 ! WF 1.10 WZ 0.95 ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 FD 0.97 GG 1.00* HN 1.02 ! KK 1.00* KP 0.97 LA 0.94 MA 1.00* ! MK 1.00* NL 1.03 ON 1.00* OV 1.03 ! PT 1.02 SC 1.03 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.05 ! ! A total of 60 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 0.97 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.11 ON 1.00* OV 1.00* ! PT 1.00* SC 1.00 TC 1.00* TS 1.00* ! WF 1.00* WZ 0.99 ! ! A total of 138 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 0.95 GG 1.00* HN 0.97 ! KK 1.00* KP 0.98 LA 0.97 MA 1.00* ! MK 1.00* NL 1.02 ON 1.00* OV 1.01 ! PT 1.04 SC 1.04 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.367528Jy sigma=0.001811 ! Fit after self-cal, rms=0.369299Jy sigma=0.001790 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7571 mas, bmaj=2.256 mas, bpa=-9.402 degrees ! Estimated noise=464.902 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00291664 Jy ! Component: 100 - total flux cleaned = 0.00292072 Jy ! Component: 150 - total flux cleaned = 0.00262491 Jy ! Component: 200 - total flux cleaned = 0.00247286 Jy ! Total flux subtracted in 200 components = 0.00247286 Jy ! Clean residual min=-0.008125 max=0.004775 Jy/beam ! Clean residual mean=-0.000037 rms=0.001305 Jy/beam ! Combined flux in latest and established models = 0.629604 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 50 components and 0.629604 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369225Jy sigma=0.001788 ! Fit after self-cal, rms=0.369571Jy sigma=0.001787 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369571Jy sigma=0.001787 ! Fit after self-cal, rms=0.369760Jy sigma=0.001773 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7574 mas, bmaj=2.255 mas, bpa=-9.352 degrees ! Estimated noise=464.807 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00378082 Jy ! Component: 100 - total flux cleaned = 0.0036601 Jy ! Component: 150 - total flux cleaned = 0.00347963 Jy ! Component: 200 - total flux cleaned = 0.00347406 Jy ! Total flux subtracted in 200 components = 0.00347406 Jy ! Clean residual min=-0.004826 max=0.003145 Jy/beam ! Clean residual mean=0.000032 rms=0.000960 Jy/beam ! Combined flux in latest and established models = 0.633078 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 53 components and 0.633078 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369681Jy sigma=0.001771 ! Fit after self-cal, rms=0.369705Jy sigma=0.001771 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000936512 Jy ! Component: 100 - total flux cleaned = 0.000875015 Jy ! Component: 150 - total flux cleaned = 0.000875593 Jy ! Component: 200 - total flux cleaned = 0.000923051 Jy ! Total flux subtracted in 200 components = 0.000923051 Jy ! Clean residual min=-0.005236 max=0.003226 Jy/beam ! Clean residual mean=0.000006 rms=0.000944 Jy/beam ! Combined flux in latest and established models = 0.634001 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 54 components and 0.634001 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369670Jy sigma=0.001770 ! Fit after self-cal, rms=0.369668Jy sigma=0.001770 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369668Jy sigma=0.001770 ! Fit after self-cal, rms=0.369465Jy sigma=0.001769 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7575 mas, bmaj=2.255 mas, bpa=-9.336 degrees ! Estimated noise=464.902 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00221218 Jy ! Component: 100 - total flux cleaned = 0.00221659 Jy ! Component: 150 - total flux cleaned = 0.00221617 Jy ! Component: 200 - total flux cleaned = 0.00226637 Jy ! Total flux subtracted in 200 components = 0.00226637 Jy ! Clean residual min=-0.004187 max=0.003128 Jy/beam ! Clean residual mean=0.000023 rms=0.000880 Jy/beam ! Combined flux in latest and established models = 0.636267 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 55 components and 0.636267 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369429Jy sigma=0.001768 ! Fit after self-cal, rms=0.369437Jy sigma=0.001768 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000460462 Jy ! Component: 100 - total flux cleaned = 0.000413314 Jy ! Component: 150 - total flux cleaned = 0.000415104 Jy ! Component: 200 - total flux cleaned = 0.000491899 Jy ! Total flux subtracted in 200 components = 0.000491899 Jy ! Clean residual min=-0.004419 max=0.003170 Jy/beam ! Clean residual mean=0.000010 rms=0.000874 Jy/beam ! Combined flux in latest and established models = 0.636759 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 61 components and 0.636759 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369413Jy sigma=0.001768 ! Fit after self-cal, rms=0.369416Jy sigma=0.001767 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369416Jy sigma=0.001767 ! Fit after self-cal, rms=0.369641Jy sigma=0.001767 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=2.433 mas, bmaj=3.511 mas, bpa=-25.08 degrees ! Estimated noise=567.635 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00170111 Jy ! Component: 100 - total flux cleaned = 0.00175238 Jy ! Component: 150 - total flux cleaned = 0.00186088 Jy ! Component: 200 - total flux cleaned = 0.00190897 Jy ! Total flux subtracted in 200 components = 0.00190897 Jy ! Clean residual min=-0.003115 max=0.002776 Jy/beam ! Clean residual mean=-0.000029 rms=0.001087 Jy/beam ! Combined flux in latest and established models = 0.638668 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 69 components and 0.638668 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369635Jy sigma=0.001767 ! Fit after self-cal, rms=0.369644Jy sigma=0.001767 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000148976 Jy ! Component: 100 - total flux cleaned = 0.000187091 Jy ! Component: 150 - total flux cleaned = 0.00021566 Jy ! Component: 200 - total flux cleaned = 0.000216617 Jy ! Total flux subtracted in 200 components = 0.000216617 Jy ! Clean residual min=-0.003118 max=0.002870 Jy/beam ! Clean residual mean=-0.000040 rms=0.001097 Jy/beam ! Combined flux in latest and established models = 0.638885 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 73 components and 0.638885 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369655Jy sigma=0.001767 ! Fit after self-cal, rms=0.369657Jy sigma=0.001767 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7576 mas, bmaj=2.255 mas, bpa=-9.321 degrees ! Estimated noise=465.112 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7576 x 2.255 at -9.321 degrees (North through East) ! Clean map min=-0.0037494 max=0.51565 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369657Jy sigma=0.001767 ! Fit after self-cal, rms=1.029876Jy sigma=0.001568 ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7563 mas, bmaj=2.255 mas, bpa=-9.365 degrees ! Estimated noise=464.485 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00133621 Jy ! Component: 100 - total flux cleaned = 0.00144456 Jy ! Component: 150 - total flux cleaned = 0.00144643 Jy ! Component: 200 - total flux cleaned = 0.0014905 Jy ! Total flux subtracted in 200 components = 0.0014905 Jy ! Clean residual min=-0.003155 max=0.002528 Jy/beam ! Clean residual mean=-0.000025 rms=0.000790 Jy/beam ! Combined flux in latest and established models = 0.640375 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 78 components and 0.640375 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.029833Jy sigma=0.001568 ! Fit after self-cal, rms=1.029850Jy sigma=0.001568 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000149927 Jy ! Component: 100 - total flux cleaned = 0.000191661 Jy ! Component: 150 - total flux cleaned = 0.000228868 Jy ! Component: 200 - total flux cleaned = 0.000228416 Jy ! Total flux subtracted in 200 components = 0.000228416 Jy ! Clean residual min=-0.003245 max=0.002494 Jy/beam ! Clean residual mean=-0.000030 rms=0.000784 Jy/beam ! Combined flux in latest and established models = 0.640603 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 79 components and 0.640604 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.029825Jy sigma=0.001568 ! Fit after self-cal, rms=1.029839Jy sigma=0.001568 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.029839Jy sigma=0.001568 ! Fit after self-cal, rms=2.447388Jy sigma=0.001567 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.5608 mas, bmaj=1.855 mas, bpa=-4.909 degrees ! Estimated noise=690.492 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.378685 Jy ! Component: 100 - total flux cleaned = 0.481697 Jy ! Component: 150 - total flux cleaned = 0.531433 Jy ! Component: 200 - total flux cleaned = 0.561593 Jy ! Total flux subtracted in 200 components = 0.561593 Jy ! Clean residual min=-0.006867 max=0.016329 Jy/beam ! Clean residual mean=0.000400 rms=0.002318 Jy/beam ! Combined flux in latest and established models = 0.561593 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.561593 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7557 mas, bmaj=2.253 mas, bpa=-9.342 degrees ! Estimated noise=464.516 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0367959 Jy ! Component: 100 - total flux cleaned = 0.054883 Jy ! Component: 150 - total flux cleaned = 0.0648315 Jy ! Component: 200 - total flux cleaned = 0.0706196 Jy ! Total flux subtracted in 200 components = 0.0706196 Jy ! Clean residual min=-0.002735 max=0.004112 Jy/beam ! Clean residual mean=0.000181 rms=0.000945 Jy/beam ! Combined flux in latest and established models = 0.632212 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 43 components and 0.632212 Jy ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Added new window around map position (-2.6, 2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00402236 Jy ! Component: 100 - total flux cleaned = 0.00627709 Jy ! Component: 150 - total flux cleaned = 0.00674219 Jy ! Component: 200 - total flux cleaned = 0.0071282 Jy ! Total flux subtracted in 200 components = 0.0071282 Jy ! Clean residual min=-0.002535 max=0.002406 Jy/beam ! Clean residual mean=-0.000016 rms=0.000759 Jy/beam ! Combined flux in latest and established models = 0.63934 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 67 components and 0.639341 Jy ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=2.427 mas, bmaj=3.506 mas, bpa=-24.93 degrees ! Estimated noise=568.966 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00157982 Jy ! Component: 100 - total flux cleaned = 0.00191617 Jy ! Component: 150 - total flux cleaned = 0.00189355 Jy ! Component: 200 - total flux cleaned = 0.00187365 Jy ! Total flux subtracted in 200 components = 0.00187365 Jy ! Clean residual min=-0.003221 max=0.002296 Jy/beam ! Clean residual mean=-0.000142 rms=0.001020 Jy/beam ! Combined flux in latest and established models = 0.641214 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.74028e-05 Jy ! Component: 100 - total flux cleaned = -5.00789e-05 Jy ! Component: 150 - total flux cleaned = -8.10437e-05 Jy ! Component: 200 - total flux cleaned = -0.000109378 Jy ! Total flux subtracted in 200 components = -0.000109378 Jy ! Clean residual min=-0.003182 max=0.002309 Jy/beam ! Clean residual mean=-0.000137 rms=0.001014 Jy/beam ! Combined flux in latest and established models = 0.641105 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 93 components and 0.641105 Jy ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.7557 mas, bmaj=2.253 mas, bpa=-9.342 degrees ! Estimated noise=464.516 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000344413 Jy ! Component: 100 - total flux cleaned = -0.000532385 Jy ! Component: 150 - total flux cleaned = -0.000531176 Jy ! Component: 200 - total flux cleaned = -0.000490449 Jy ! Total flux subtracted in 200 components = -0.000490449 Jy ! Clean residual min=-0.002529 max=0.002458 Jy/beam ! Clean residual mean=-0.000053 rms=0.000733 Jy/beam ! Combined flux in latest and established models = 0.640614 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 104 components and 0.640615 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=2.447331Jy sigma=0.001566 ! Fit after self-cal, rms=2.447284Jy sigma=0.001566 wmodel J0239+0416_X_2003_06_18_pus_map.mod ! Writing 104 model components to file: J0239+0416_X_2003_06_18_pus_map.mod wobs J0239+0416_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J0239+0416_X_2003_06_18_pus_uvs.fits wwins J0239+0416_X_2003_06_18_pus_map.win ! wwins: Wrote 3 windows to J0239+0416_X_2003_06_18_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000741695 Jy ! Component: 100 - total flux cleaned = -0.000913614 Jy ! Component: 150 - total flux cleaned = -0.000992792 Jy ! Component: 200 - total flux cleaned = -0.00106784 Jy ! Component: 250 - total flux cleaned = -0.00110407 Jy ! Component: 300 - total flux cleaned = -0.00106897 Jy ! Component: 350 - total flux cleaned = -0.00100061 Jy ! Component: 400 - total flux cleaned = -0.000933668 Jy ! Component: 450 - total flux cleaned = -0.000868654 Jy ! Component: 500 - total flux cleaned = -0.000804814 Jy ! Component: 550 - total flux cleaned = -0.000742239 Jy ! Component: 600 - total flux cleaned = -0.00058988 Jy ! Component: 650 - total flux cleaned = -0.00053038 Jy ! Component: 700 - total flux cleaned = -0.000530204 Jy ! Component: 750 - total flux cleaned = -0.000472175 Jy ! Component: 800 - total flux cleaned = -0.00041559 Jy ! Component: 850 - total flux cleaned = -0.000387791 Jy ! Component: 900 - total flux cleaned = -0.000333011 Jy ! Component: 950 - total flux cleaned = -0.000279008 Jy ! Component: 1000 - total flux cleaned = -0.000199488 Jy ! Total flux subtracted in 1024 components = -0.000173422 Jy ! Clean residual min=-0.001303 max=0.001688 Jy/beam ! Clean residual mean=-0.000023 rms=0.000536 Jy/beam ! Combined flux in latest and established models = 0.640441 Jy keep ! Adding 59 model components to the UV plane model. ! The established model now contains 163 components and 0.640441 Jy wmap "J0239+0416_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7557 x 2.253 at -9.342 degrees (North through East) ! Clean map min=-0.002328 max=0.51383 Jy/beam ! Writing clean map to FITS file: J0239+0416_X_2003_06_18_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.513833 invert ! Inverting map ! Your choice of large map pixels excluded 0.738% of the data. ! The x-axis pixel size should ideally be below 0.1778 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000534088 device "J0239+0416_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J0239+0416_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.311826 0.311826 0.623651 1.2473 2.49461 4.98921 9.97842 19.9568 39.9137 79.8274 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.513 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7557 x 2.253 at -9.342 degrees (North through East) ! Clean map min=-0.002328 max=0.51383 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0239+0416_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J0239+0416_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J0239+0416_X_2003_06_18_pus_uvs.log closed on Wed Jan 17 16:19:06 2007